Data processing assessment for the Lunar Geoscience Observer imaging spectrometer

Details Data processing assessment for the Lunar Geoscience Observer imaging spectrometer Data processing assessment for the Lunar Geoscience Observer imaging spectrometer

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988spie..890..152i&link_type=abstract

IN: Infrared systems and components II; Proceedings of the Meeting, Los Angeles, CA, Jan. 14, 15, 1988 (A89-15891 04-32). Bellin

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Lunar Probes, Spectrometers, Data Reduction, Infrared Spectrometers, Lunar Surface, Pixels, Visible Spectrum

Scientific paper

On the Lunar Geoscience Observer project, a Visible and Infrared Mapping Spectrometer instrument has been proposed. This instrument will have science data input rates in the hundreds of kilobits per second (kbps) and an average telemetry output data rate of 4 kbps. Techniques that can be used to reduce the throughput of the instrument are editing, summing and averaging, data compression, data preprocessing, pattern recognition and snapshot data taking. Due to instrument limitations in the buffer memory size and processing speeds, a careful selection of the available techniques must be made.

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